{"id":9299,"date":"2024-07-11T14:47:56","date_gmt":"2024-07-11T18:47:56","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=9299"},"modified":"2024-07-11T14:47:56","modified_gmt":"2024-07-11T18:47:56","slug":"scientific-definition-of-a-planet-says-it-must-orbit-our-sun-a-new-proposal-would-change-that","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=9299","title":{"rendered":"Scientific Definition of a Planet Says It Must Orbit Our Sun; A New Proposal Would Change That"},"content":{"rendered":"<figure style=\"width: 1170px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium lazyload\" data-src=\"https:\/\/s3.amazonaws.com\/cms.ipressroom.com\/173\/files\/20246\/6684fe202cfac2492947efe9_Solar+System+2\/Solar+System+2_hero.jpg\" width=\"1170\" height=\"780\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 1170px; --smush-placeholder-aspect-ratio: 1170\/780;\"><figcaption class=\"wp-caption-text\">CactiStaccingCrane\/Wikimedia Commons<\/figcaption><\/figure>\n<p><strong>Key takeaways<\/strong><\/p>\n<ul>\n<li>The International Astronomical Union defines a planet as a celestial body that orbits the sun, is massive enough that gravity has forced it into a spherical shape, and has cleared away other objects near its orbit around the sun.&nbsp;<\/li>\n<li>Scientists now recognize the existence of thousands of planets, but the IAU definition applies only to those within our solar system.<\/li>\n<li>The new proposed definition specifies that the body may orbit one or more stars, brown dwarfs or stellar remnants and sets mass limits that should apply to planets everywhere.<\/li>\n<\/ul>\n<p>Planetary scientists are proposing a new definition of a planet to replace one that many researchers view as sun-centric and outdated. The current definition \u2014 established in 2006 by the International Astronomical Union, or IAU, the organization that officially names objects in space \u2014 specifies that to qualify as a planet, a celestial body must orbit the sun within our solar system.<\/p>\n<p>But scientists know that celestial bodies orbiting stars outside our solar system are fairly common, and a forthcoming article in the&nbsp;<em><a href=\"http:\/\/arxiv.org\/abs\/2407.07590\" target=\"_blank\" rel=\"noopener\">Planetary Science Journal<\/a><\/em>&nbsp;argues for a new definition of a planet that includes being unrestrained by the bounds of our solar system. The proposal also provides quantitative criteria to further clarify the definition of a planet.&nbsp;<\/p>\n<p>Jean-Luc Margot, lead author of the article and UCLA professor of earth, planetary and space sciences and of physics and astronomy, will present the proposed new definition at the IAU General Assembly in August 2024.<\/p>\n<p>Under the current definition, a planet is a celestial body that orbits the sun, is massive enough that gravity has forced it into a spherical shape, and has cleared away other objects near its orbit around the sun.&nbsp;<\/p>\n<p>\u201cThe current definition specifically mentions orbiting our sun. We now know about the existence of thousands of planets, but the IAU definition applies only to the ones in our solar system,\u201d Margot said. We propose a new definition that can be applied to celestial bodies that orbit any star, stellar remnant or brown dwarf.\u201d<\/p>\n<p>The authors argue that while the requirement to orbit our sun is too specific, other criteria in the IAU definition are too vague. For example, it says a planet has \u201ccleared its orbit\u201d without stating what that means. The proposed new definition contains quantifiable criteria that can be applied for defining planets inside and outside our solar system.<\/p>\n<p>In the new definition, a planet is a celestial body that:<\/p>\n<ul>\n<li>orbits one or more stars, brown dwarfs or stellar remnants and<\/li>\n<li>is more massive than 10<sup>23<\/sup>&nbsp;kg and<\/li>\n<li>is less massive than 13 Jupiter masses (2.5 X 10<sup>28<\/sup>&nbsp;kg).<\/li>\n<\/ul>\n<p>Margot and co-authors Brett Gladman of the University of British Columbia and Tony Yang, a student at Chaparral High School in Temecula, California, ran a mathematical algorithm on the properties of objects in our solar system to see which objects clustered together. The analysis revealed groups of distinct qualities shared by planets in our solar system that can be used as a starting point for creating a taxonomy for planets in general.&nbsp;<\/p>\n<p>For example, if an object has enough gravity to clear a path by accumulating or ejecting smaller objects nearby, it is said to be dynamically dominant.&nbsp;<\/p>\n<p>\u201cAll the planets in our solar system are dynamically dominant, but other objects \u2014 including dwarf planets like Pluto, which is not a true planet, and asteroids \u2014 are not,\u201d Margot said. \u201cSo this property can be included in the definition of planet.\u201d<\/p>\n<p>The requirement for dynamical dominance provides a lower limit on mass. But potential planets can also be too big to fit the new definition. Some gas giants, for example, are so large that thermonuclear fusion of deuterium occurs, and the object becomes a substar called a brown dwarf and therefore not a planet. This limit has been determined to be the mass of 13 or more Jupiters.&nbsp;<\/p>\n<p>The current requirement to be spherical, on the other hand, is more problematic. Distant planets can rarely be observed in enough detail to ascertain their shape with certainty. The authors argue that the shape requirement is so difficult to implement that it is effectively useless for definitional purposes, even though planets are generally round.&nbsp;<\/p>\n<p>\u201cHaving definitions anchored to the most easily measurable quantity \u2014 mass \u2014 removes arguments about whether or not a specific object meets the criterion,\u201d Gladman said. \u201cThis is a weakness of the current definition.\u201d<\/p>\n<p>The good news is that, in the solar system, celestial bodies larger than 10<sup>21<\/sup>&nbsp;kg appear to be round. So all bodies that satisfy the proposed lower limit on mass of 10<sup>23<\/sup>&nbsp;kg are expected to be spherical.<\/p>\n<p>While any official change to the IAU definition of planet is likely a few years away, Margot and his colleagues hope their work starts a conversation that results in an improved definition.<\/p>\n<p><em>&#8211; Holly Ober, UCLA<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Key takeaways The International Astronomical Union defines a planet as a celestial body that orbits the sun, is massive enough that gravity has forced it into a spherical shape, and has cleared away other objects near its orbit around the sun.&nbsp; Scientists now recognize the existence of thousands of planets, but the IAU definition applies&hellip;<\/p>\n","protected":false},"author":71,"featured_media":9300,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/s3.amazonaws.com\/cms.ipressroom.com\/173\/files\/20246\/6684fe202cfac2492947efe9_Solar+System+2\/Solar+System+2_hero.jpg","fifu_image_alt":"Scientific Definition of a Planet Says It Must Orbit Our Sun; A New Proposal Would Change That","footnotes":""},"categories":[207],"tags":[],"class_list":["post-9299","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-research"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9299","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=9299"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9299\/revisions"}],"predecessor-version":[{"id":9301,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9299\/revisions\/9301"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/9300"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=9299"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=9299"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=9299"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}